Association between Super- nova Remnants and Stellar Formation

DUVIDOVICH, L.; ORTEGA M.; SALDANO H.; CELIS M.

Congreso; Segunda Reunion Binacional AAA-SOCHIAS; 2018

The supernova remnants (SNRs) provide much of the energy that heats up the interstellar medium(ISM) and their shock waves can accelerate, compress, heat, fragment (or even destroy) surrounding interstellarclouds, possibly leading to the formation of a new generation of stars. SNRs are often not far away from theirnatal giant molecular clouds (MCs), and in many cases, both would be in physical contact, as is expected. Theinteraction between SNRs and dense interstellar clouds could be characterized by the infrared, sub-millimetreand radio emissions study. We carried out a preliminary analysis towards two supernova remnants wrapped incomplex interstellar mediums, which present diverse HII regions and young stellar objects. We discuss here boththe SNR-MC association through the relationship of the dusty clump parameters with those of the radio emissionscoming from SNRs and also the likely scenarios of star formation. This study may open the possibility for futureAPEX and ALMA (band-5 and 7) observations which will allow us to have a more detailed knowledge about suchSNR-MC interaction.